GOALS-JWST: resolved multiphase molecular gas in IRAS 20551-4250 using JWST and ALMA
Studying the content and distribution of molecular gas (H $_{2}$) provides key insights into how feedback from active galactic nuclei (AGNs) and star formation influences galaxy evolution, since molecular gas is the primary fuel for star formation. Ultra-luminous infrared galaxies (ULIRGs) are ideal candidates to study how AGNs and/or starbursts
Kakkad, D. et al.
Fecha de publicación:
6
2026